Please use this identifier to cite or link to this item: https://olympias.lib.uoi.gr/jspui/handle/123456789/17282
Full metadata record
DC FieldValueLanguage
dc.contributor.authorAlissandrakis, C. E.en
dc.date.accessioned2015-11-24T18:38:07Z-
dc.date.available2015-11-24T18:38:07Z-
dc.identifier.issn0273-1177-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/17282-
dc.rightsDefault Licence-
dc.titleRadio observations of the quiet solar coronaen
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.primaryhttp://dx.doi.org/10.1016/0273-1177(94)90167-8-
heal.identifier.secondaryhttp://www.sciencedirect.com/science/article/pii/0273117794901678-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate1994-
heal.abstractObservations of radio emission from the quiet solar atmosphere and the associated emission mechanisms are discussed. Long wavelength observations, with a spatial resolution of ?1 arc min are ideal for the study of the large scale structure of the corona, including coronal holes, arches, streamers and the base of the heliospheric current sheet. These structures are observed both beyond the limb and on the solar disk, with little line of sight integration. We also discuss diagnostics of electron temperature and density, as well as the interpretation problems arising from the inhomogeneity of the corona and refraction effects.en
heal.journalNameAdvances in Space Researchen
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά)

Files in This Item:
File Description SizeFormat 
alissandrakis-1994-Radio observations of the quiet solar corona.pdf774.04 kBAdobe PDFView/Open    Request a copy


This item is licensed under a Creative Commons License Creative Commons